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The Astrophysical Journal, 728:65 (6pp), 2011 February 10 doi:10.1088/0004-637X/728/1/65 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary: The Astrophysical Journal, 728:65 (6pp), 2011 February 10 doi:10.1088/0004-637X/728/1/65
C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
FILAMENT INTERACTION MODELED BY FLUX ROPE RECONNECTION
T. T¨or¨ok1,2
, R. Chandra1,3
, E. Pariat1
, P. D´emoulin1
, B. Schmieder1
, G. Aulanier1
, M. G. Linton4
, and C. H. Mandrini5
1 LESIA, Observatoire de Paris, CNRS, UPMC, Universit´e Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France
2 Predictive Science, Inc., 9990 Mesa Rim Rd., Ste. 170, San Diego, CA 92121, USA
3 Department of Physics, DSB Campus, Kumaun University, Naini Tal 263 002, Uttarakhand, India
4 Naval Research Laboratory, Washington, DC, 20375 USA
5 Instituto de Astronom´ia y F´isica del Espacio (IAFE), CONICET-UBA, and Facultad de Ciencias Exactas y Naturales (FCEN), UBA, Buenos Aires, Argentina
Received 2010 September 16; accepted 2010 December 8; published 2011 January 20
ABSTRACT
H observations of solar active region NOAA 10501 on 2003 November 20 revealed a very uncommon dynamic
process: during the development of a nearby flare, two adjacent elongated filaments approached each other, merged

  

Source: Aulanier, Guillaume - Observatoire de Paris
Demoulin, Pascal - Observatoire de Paris

 

Collections: Physics